Описание: This concise and systematic account of the current state of this new branch of astrophysics presents the theoretical foundations of plasma astrophysics, magneto-hydrodynamics and coronal magnetic structures, taking into account the full range of available observation techniques -- from radio to gamma.
Автор: Tim Howard Название: Space Weather and Coronal Mass Ejections ISBN: 1461479746 ISBN-13(EAN): 9781461479741 Издательство: Springer Рейтинг: Цена: 7182.00 р. Наличие на складе: Есть у поставщика Поставка под заказ.
Описание: In this SpringerBrief, Space Weather and Coronal Mass Ejections, author Timothy Howard briefly introduces the coronal mass ejection, its scientific importance, and its relevance to space weather at Earth and other planets.
Автор: Timothty Howard Название: Coronal Mass Ejections ISBN: 1461428793 ISBN-13(EAN): 9781461428794 Издательство: Springer Рейтинг: Цена: 19589.00 р. Наличие на складе: Есть у поставщика Поставка под заказ.
Описание: Coronal Mass Ejections provides an introduction to the solar coronal mass ejection phenomena. Readers will find a discussion of both corona and interplanetary coronal mass ejections, while learning how to detect and extract data from them.
Автор: Steven Tomczyk; Jie Zhang; Timothy Bastian Название: Coronal Magnetometry ISBN: 1493920375 ISBN-13(EAN): 9781493920372 Издательство: Springer Рейтинг: Цена: 15672.00 р. Наличие на складе: Есть у поставщика Поставка под заказ.
Описание: Captures advances being made in the field of coronal magnetism, from theory to observations and instrumentation.This volume is a collection of research articles on the subject of the solar corona, and particularly, coronal magnetism.
Автор: David Burgess; James Drake; Eckart Marsch; Rudolf Название: Multi-Scale Physics in Coronal Heating and Solar Wind Acceleration ISBN: 1461464609 ISBN-13(EAN): 9781461464600 Издательство: Springer Рейтинг: Цена: 20896.00 р. Наличие на складе: Есть у поставщика Поставка под заказ.
Описание: This volume explores the cross-linkages between the kinetic processes and macroscopic phenomena in the solar atmosphere, which are at the heart of our current understanding of the heating of the closed and open corona and the acceleration of the solar wind.
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